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Long Periods in the Three-Dimensional Motion of Trojan Asteroids

  • R. Bien (a1) and J. Schubart (a1)
Abstract

The long periods caused by Jupiter, or Jupiter and Saturn in the motion of a Trojan are studied by numerical integration. Orbital inclinations between 0° and 50° are considered. Results on the length of the periods and on their main effects in the osculating elements are presented. It turns out that secular resonances can be important for the evolution of Trojan orbits.

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Copyright
COPYRIGHT: © Reidel 1983
References
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Bien, R. : 1980a, Astron.Astrophys. 81, pp.255–259.
Bien, R. : 1980b, Moon and Planets 22, pp.163–166.
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Cohen, C.J., Hubbard, E.C., and Oesterwinter, C.: 1973, Astron. Papers American Ephemeris Washington, Vol.22, part 1.
Érdi, B. : 1981, Celes.Mech. 24, pp.377–390.
Schubart, J. : 1978, Dynamics of Planets and Satellites and Theories of their Motion, Ed.: Szebehely, V. IAU Coll. No.41, pp.137–143.
Schubart, J. : 1979, Dynamics of the Solar System, Ed.: Duncombe, R.L. IAU Symp. No.81, pp.207–215.
Schubart, J. and Stumpff, P.: 1966, Veroeffentl.Astron. Rechen-Inst. Heidelberg No.18.
Yoder, C.F.: 1979, Icarus 40, pp.341–344.
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Proceedings of the International Astronomical Union
  • ISSN: -
  • EISSN: 0252-9211
  • URL: /core/journals/proceedings-of-the-international-astronomical-union
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